F
Fabian Walter
Researcher at Max Planck Society
Publications - 1053
Citations - 92179
Fabian Walter is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 146, co-authored 999 publications receiving 83016 citations. Previous affiliations of Fabian Walter include California Institute of Technology & University of Bonn.
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The ngVLA science case and associated science requirements
Eric J. Murphy,Alberto D. Bolatto,Shami Chatterjee,Caitlin M. Casey,Laura Chomiuk,Daniel A. Dale,I. de Pater,Mark Dickinson,James Di Francesco,James Di Francesco,Gregg Hallinan,A. Isella,Kotaro Kohno,Shrinivas R. Kulkarni,Cornelia C. Lang,T. J. W. Lazio,Adam K. Leroy,Laurent Loinard,Thomas J. Maccarone,Brenda C. Matthews,Brenda C. Matthews,Rachel A. Osten,Mark J. Reid,Dominik Riechers,Nami Sakai,Fabian Walter,David J. Wilner +26 more
Posted Content
Spatially resolved kinematics of the multi-phase interstellar medium in the inner disk of M82
TL;DR: In this article, the authors present spatially resolved kinematics of the interstellar NaI D 5890,5896 doublet absorption and 12CO(1-0) emission across the inner 2 × 1 kpc of the disk of M82.
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HI and Hot Gas in the Outskirts of the M81 Group
TL;DR: In this paper, a high-resolution HI synthesis survey of the outer regions of the nearby M81 group is presented, where internal (galactic) and external (group-related) evolution processes can be studied simultaneously in great detail.
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Polycyclic Aromatic Hydrocarbon and Mid-Infrared Continuum Emission in a z>4 Submillimeter Galaxy
Dominik A. Riechers,Dominik A. Riechers,Alexandra Pope,Emanuele Daddi,Lee Armus,Chris Carilli,Fabian Walter,Jacqueline Hodge,Ranga-Ram Chary,Glenn Morrison,Mark Dickinson,Helmut Dannerbauer,David Elbaz +12 more
TL;DR: In this paper, the authors reported the detection of 6.2um polycyclic aromatic hydrocarbons (PAH) and rest-frame 4-7um continuum emission in the z=4.055 submillimeter galaxy GN20, using the Infrared Spectrograph (IRS) on board the Spitzer Space Telescope.
Posted Content
Dust May Be More Rare Than Expected in Metal Poor Galaxies
David B. Fisher,Alberto D. Bolatto,Rodrigo Herrera-Camus,Bruce T. Draine,J. Donaldson,Fabian Walter,Karin Sandstrom,Adam K. Leroy,John M. Cannon,Karl D. Gordon +9 more
TL;DR: In this article, the authors reported observations of dust emission from I Zw 18 from which they determined its dust mass to be 450-1800 Msun, yielding a dust-to-stellar mass ratio of 3.2-13x10-6.